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Many galaxies are chock-full of dust,
while others have occasional dark streaks of opaque cosmic soot swirling
in amongst their gas and stars. However, the subject of this new image,
snapped with the OmegaCAM camera on ESO’s VLT Survey Telescope in
Chile, is unusual — the small galaxy, named IC 1613, is a veritable
clean freak! IC 1613 contains very little cosmic dust, allowing
astronomers to explore its contents with great clarity. This is not just
a matter of appearances; the galaxy’s cleanliness is vital to our
understanding of the Universe around us.
IC 1613 is a dwarf galaxy in the constellation of Cetus (The Sea Monster). This VST image  shows the galaxy’s unconventional beauty, all scattered stars and bright pink gas, in great detail.
German astronomer Max Wolf discovered IC 1613’s faint glow in 1906. In 1928, his compatriot Walter Baade used the more powerful 2.5-metre telescope at the Mount Wilson Observatory
in California to successfully make out its individual stars. From these
observations, astronomers figured out that the galaxy must be quite
close to the Milky Way, as it is only possible to resolve single
pinprick-like stars in the very nearest galaxies to us.
Astronomers have since confirmed that IC 1613 is indeed a member of the Local Group,
a collection of more than 50 galaxies that includes our home galaxy,
the Milky Way. IC 1613 itself lies just over 2.3 million light-years
away from us. It is relatively well-studied due to its proximity;
astronomers have found it to be an irregular dwarf that lacks many of
the features, such as a starry disc, found in some other diminutive
However, what IC 1613 lacks in form, it makes up for in tidiness. We
know IC 1613’s distance to a remarkably high precision, partly due to
the unusually low levels of dust lying both within the galaxy and along
the line of sight from the Milky Way — something that enables much
clearer observations .
The second reason we know the distance to IC 1613 so precisely is that the galaxy hosts a number of notable stars of two types: Cepheid variables and RR Lyrae variables. Both types of star rhythmically pulsate, growing characteristically bigger and brighter at fixed intervals (eso1311).
As we know from our daily lives on Earth, shining objects such as
light bulbs or candle flames appear dimmer the further they are away
from us. Astronomers can use this simple piece of logic to figure out
exactly how far away things are in the Universe— so long as they know
how bright they really are, referred to as their intrinsic brightness.
Cepheid and RR Lyrae variables have the special property that their
period of brightening and dimming is linked directly to their intrinsic
brightness. So, by measuring how quickly they fluctuate astronomers can
work out their intrinsic brightness. They can then compare these values
to their apparent measured brightness and work out how far away they
must be to appear as dim as they do.
Stars of known intrinsic brightness can act like standard candles,
as astronomers say, much like how a candle with a specific brightness
would act as a good gauge of distance intervals based on the observed
brightness of its flame’s flicker.
Using standard candles — such as the variable stars within IC 1613 and the less-common Type Iasupernova explosions, which can seen across far greater cosmic distances — astronomers have pieced together a cosmic distance ladder, reaching deeper and deeper into space.
Decades ago, IC 1613 helped astronomers work out how to utilise
variable stars to chart the Universe’s grand expanse. Not bad for a
little, shapeless galaxy.
 OmegaCAM is a 32-CCD, 256-million-pixel camera mounted on the
2.6-metre VLT Survey Telescope at Paranal Observatory in Chile.Click hereto view more images taken by OmegaCAM.
 Cosmic dust is made of various
heavier elements, such as carbon and iron, as well as larger, grainier
molecules. Not only does dust block out light, making dust-shrouded
objects harder to see, it also preferentially scatters bluer light. As a
result, cosmic dust makes objects appear redder when seen through our
telescopes than they are in reality. Astronomers can factor out thisreddeningwhen studying objects. Still, the less reddening, the more precise an observation is likely to be.
 Other than the twoMagellanic Clouds, IC 1613 is the only irregular dwarf galaxy in the Local Group in which RR Lyrae type variable stars have been identified.
ESO is the foremost intergovernmental astronomy organisation in Europe
and the world’s most productive ground-based astronomical observatory by
far. It is supported by 16 countries: Austria, Belgium, Brazil, the
Czech Republic, Denmark, France, Finland, Germany, Italy, the
Netherlands, Poland, Portugal, Spain, Sweden, Switzerland and the United
Kingdom, along with the host state of Chile. ESO carries out an
ambitious programme focused on the design, construction and operation of
powerful ground-based observing facilities enabling astronomers to make
important scientific discoveries. ESO also plays a leading role in
promoting and organising cooperation in astronomical research. ESO
operates three unique world-class observing sites in Chile: La Silla,
Paranal and Chajnantor. At Paranal, ESO operates the Very Large
Telescope, the world’s most advanced visible-light astronomical
observatory and two survey telescopes. VISTA works in the infrared and
is the world’s largest survey telescope and the VLT Survey Telescope is
the largest telescope designed to exclusively survey the skies in
visible light. ESO is a major partner in ALMA, the largest astronomical
project in existence. And on Cerro Armazones, close to Paranal, ESO is
building the 39-metre European Extremely Large Telescope, the E-ELT,
which will become “the world’s biggest eye on the sky”.